HIP 855
HIP 855 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,463 light-years, HIP 855 is a distant star lying deep within the Milky Way galaxy.
HIP 855 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 855 has an apparent magnitude of +7.75, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its red hue, which corresponds to a B-V color index of +1.487.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,487 |
Observation
| Magnitude Apparente | +7.75 |
| Magnitude Absolue | -0,51 |
| Distance | 1,463 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 10,48m |
| Déclinaison | 51° 54,74′ |
Frequently Asked Questions
What type of star is HIP 855?
HIP 855 is a Class K — K-type (Orange) star.
How far is HIP 855 from Earth?
HIP 855 is approximately 1,462.6 light-years from Earth.
Can you see HIP 855 with the naked eye?
With an apparent magnitude of 7.75, HIP 855 is not visible to the naked eye.
What constellation is HIP 855 in?
HIP 855 is located in the constellation Cassiopeia.